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AbstractAbstract
[en] The formation of the spatial structure of planetary nebulae with binary central stars is considered. It is shown that the main structure (the enhanced density area) has the form of an hour-glass or a toroid. The peripheral structure (a relatively fainter shell around the main structure) has the form of an ablate spheroid. If a planetary nebula is ionised incompletely, the observed form a peripheral structure can differ from the real form of an envelope
Original Title
Prostranstvennaya struktura planetarnykh tumannostej s dvojnymi yadrami
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Source
1986; 7 p; 11 refs.; 4 figs.
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Report
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